A speed limit on tachyon fields from cosmological and fine-structure data
J. D. F. Dias, Nils Sch\"oneberg, L\'eo Vacher, C. J. A. P. Martins,, Samy Vinzl

TL;DR
This paper constrains the rolling tachyon model using cosmological and fine-structure data, showing most evolutions are excluded and that the model behaves like a cosmological constant or test field.
Contribution
It provides the first comprehensive constraints on the tachyon model from combined cosmological and fine-structure measurements.
Findings
|1+w_0| < 10^{-3} from cosmology
|1+w_0| < 10^{-9} from fine-structure data
Most allowed evolutions are slow and resemble a cosmological constant
Abstract
The rolling tachyon is a non-canonical scalar field model well motivated in string theory which naturally predicts variations of the fine-structure constant. Such variations can in principle lead to interesting observable consequences, but they can also lead to extremely tight constraints on these kinds of models. In this work we subject the rolling tachyon model evolving in a variety of potentials to current data and show that most cosmologically interesting evolutions are already strongly excluded. We find from cosmological data and from fine-structure data, leaving the rolling tachyon to either play a role almost entirely equivalent to a cosmological constant or that of a test field. We also find that in most of the allowed parameter space the field evolves very slowly, allowing its evolution to be approximated as an equivalent canonical scalar…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCosmology and Gravitation Theories · Geophysics and Gravity Measurements · Scientific Research and Discoveries
